Search Publications

Weighing stars from birth to death: mass determination methods across the HRD
DOI: 10.1007/s00159-021-00132-9 Bibcode: 2021A&ARv..29....4S

Feuillet, Diane K.; Girardi, Léo; Stassun, Keivan G. +31 more

The mass of a star is the most fundamental parameter for its structure, evolution, and final fate. It is particularly important for any kind of stellar archaeology and characterization of exoplanets. There exist a variety of methods in astronomy to estimate or determine it. In this review we present a significant number of such methods, beginning …

2021 Astronomy and Astrophysics Review
Gaia 73
Time-resolved spectroscopy and photometry of M dwarf flare star YZ Canis Minoris with OISTER and TESS: Blue asymmetry in the Hα line during the non-white light flare
DOI: 10.1093/pasj/psaa098 Bibcode: 2021PASJ...73...44M

Notsu, Yuta; Kowalski, Adam F.; Maehara, Hiroyuki +15 more

In this paper, we present the results from spectroscopic and photometric observations of the M-type flare star YZ CMi in the framework of the Optical and Infrared Synergetic Telescopes for Education and Research (OISTER) collaborations during the Transiting Exoplanet Survey Satellite (TESS) observation period. We detected 145 white-light flares fr…

2021 Publications of the Astronomical Society of Japan
Gaia 72
Infrared observations of the flaring maser source G358.93-0.03. SOFIA confirms an accretion burst from a massive young stellar object
DOI: 10.1051/0004-6361/202039645 Bibcode: 2021A&A...646A.161S

Menten, K. M.; Eislöffel, J.; Klose, S. +24 more

Context. Class II methanol masers are signposts of massive young stellar objects (MYSOs). Recent evidence shows that flares of these masers are driven by MYSO accretion bursts. Thus, maser monitoring can be used to identify such bursts which are hard to discover otherwise. Infrared observations reveal burst-induced changes in the spectral energy d…

2021 Astronomy and Astrophysics
AKARI Herschel ISO 72
Stellar migration and chemical enrichment in the milky way disc: a hybrid model
DOI: 10.1093/mnras/stab2718 Bibcode: 2021MNRAS.508.4484J

Quinn, Thomas R.; Weinberg, David H.; Christensen, Charlotte R. +6 more

We develop a hybrid model of galactic chemical evolution that combines a multiring computation of chemical enrichment with a prescription for stellar migration and the vertical distribution of stellar populations informed by a cosmological hydrodynamic disc galaxy simulation. Our fiducial model adopts empirically motivated forms of the star format…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 72
A Diversity of Wave-driven Presupernova Outbursts
DOI: 10.3847/1538-4357/abc87c Bibcode: 2021ApJ...906....3W

Fuller, Jim; Wu, Samantha

Many core-collapse supernova (SN) progenitors show indications of enhanced pre-SN mass loss and outbursts, some of which could be powered by wave energy transport within the progenitor star. Depending on the star's structure, convectively excited waves driven by late-stage nuclear burning can carry substantial energy from the core to the envelope,…

2021 The Astrophysical Journal
eHST 72
The Broadband Counterpart of the Short GRB 200522A at z = 0.5536: A Luminous Kilonova or a Collimated Outflow with a Reverse Shock?
DOI: 10.3847/1538-4357/abc74a Bibcode: 2021ApJ...906..127F

Berger, E.; Cucchiara, A.; Dong, Y. +20 more

We present the discovery of the radio afterglow and near-infrared (NIR) counterpart of the Swift short gamma-ray burst (GRB) GRB 200522A, located at a small projected offset of ≈1 kpc from the center of a young, star-forming host galaxy at z = 0.5536. The radio and X-ray luminosities of the afterglow are consistent with those of on-axis cosmologic…

2021 The Astrophysical Journal
eHST 72
On the Three-dimensional Structure of Local Molecular Clouds
DOI: 10.3847/1538-4357/ac1f96 Bibcode: 2021ApJ...919...35Z

Koch, Eric W.; Alves, João; Speagle, Joshua S. +9 more

We leverage the 1 pc spatial resolution of the Leike et al. three-dimensional (3D) dust map to characterize the 3D structure of nearby molecular clouds (d ≲ 400 pc). We start by "skeletonizing" the clouds in 3D volume density space to determine their "spines," which we project on the sky to constrain cloud distances with ≈1% uncertainty. For each …

2021 The Astrophysical Journal
Gaia 72
Probabilistic Association of Transients to their Hosts (PATH)
DOI: 10.3847/1538-4357/abe8d2 Bibcode: 2021ApJ...911...95A

Prochaska, J. Xavier; Deller, Adam T.; Tendulkar, Shriharsh P. +4 more

We introduce a new method to estimate the probability that an extragalactic transient source is associated with a candidate host galaxy. This approach relies solely on simple observables: sky coordinates and their uncertainties, galaxy fluxes, and angular sizes. The formalism invokes Bayes' rule to calculate the posterior probability $P\left({O}_{…

2021 The Astrophysical Journal
eHST 72
Early-time Light Curves of Type Ia Supernovae Observed with TESS
DOI: 10.3847/1538-4357/abcd42 Bibcode: 2021ApJ...908...51F

Pál, András; Kochanek, C. S.; Latham, David W. +19 more

We present the early-time light curves of Type Ia supernovae (SNe Ia) observed in the first six sectors of Transiting Exoplanet Survey Satellite (TESS) data. Ten of these SNe were discovered by ASAS-SN, seven by ATLAS, six by ZTF, and one by Gaia. For nine of these objects with sufficient dynamic range (>3.0 mag from detection to peak), we fit …

2021 The Astrophysical Journal
Gaia 71
The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
DOI: 10.3847/1538-4357/abcec1 Bibcode: 2021ApJ...907...17L

Williams, Benjamin F.; Zezas, Andreas; Basu-Zych, Antara +7 more

In this work, we present detailed constraints on the metallicity dependence of the high-mass X-ray binary (HMXB) X-ray luminosity function (XLF). We analyze ≈5 Ms of Chandra data for 55 actively star-forming galaxies at D ≲ 30 Mpc, with gas-phase metallicities spanning $12+\mathrm{log}({\rm{O}}/{\rm{H}})$ ≈ 7-9.2. Within the galactic footprints, o…

2021 The Astrophysical Journal
Herschel 71